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Second order scalar perturbations induced by primordial curvature and tensor perturbations


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Second order scalar perturbations induced by primordial curvature and tensor perturbations by Zhe Changa et al. on Wednesday 23 November
The primordial perturbations will inevitably generate higher order
perturbations. We study the second order scalar perturbations generated by the
primordial curvature and tensor perturbations in the radiation-dominated era.
After presenting all the possible second-order source terms, we obtain the
explicit expressions of the kernel functions and the power spectra of the
second order scalar perturbations. The contributions from the initial
second-order perturbations are considered. We calculate the power spectra of
second order scalar perturbations for different tensor-to-scalar ratio $r$.
arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.11948v1
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Astro arXiv | all categoriesBy Corentin Cadiou